Stereo Pairs 
An explanation of stereo pairs and their use (PDF)  

Planned stereo pairs have suitable stereo convergence angles and illumination by design. In addition to planned stereo pairs, the Pairendipity software can identify overlapping HiRISE images that are serendipitously suitable for stereo processing and find stereo pairs within the CTX dataset.

Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below. Since this list is based on produced stereo anaglyphs it also contains a few serendipitous pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed in the “Pairendipity Stereo” link, while CTX stereo pairs are listed in “Pairendipity CTX Stereo”.

Images taken close together in time minimize illumination and frost differences and are especially useful (see the Delta-Days column in the Pairendipity files or difference the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.

Possible Phyllosilicates in Southern Argyre Planitia:   ESP_024386_1235   ESP_085798_1235   (Interval in Earth days: 4785)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-56.1

314.

7.85

-7.17

69.3

66.3

Apollinaris Sulci Indurated Dunes:   ESP_024483_1675   ESP_024127_1675   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.6

178.

23.0

6.505

40.2

37.0

Dune Composition:   ESP_025042_1375   ESP_024976_1375   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.3

42.0

0.35

18.39

69.4

67.5

Meanders and Tributaries in Ridge Form in the Zephyria Region:   ESP_024484_1750   ESP_024985_1750   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.09

151.

4.43

19.16

38.5

43.0

Lava Coating, Flood-Carved Kasei Valles:   ESP_024202_2010   ESP_024703_2010   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.84

287.

-2.9

19.15

38.0

35.7

The Eastern Floor of Aram Chaos:   ESP_024266_1830   ESP_023910_1830   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.112

340.

24.6

9.188

33.0

32.9

Dunes:   ESP_024060_1205   ESP_023928_1205   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-59.1

218.

-18.

5.39

67.4

63.9

Possible MSL Rover Landing Site in Gale Crater:   ESP_024102_1755   ESP_025368_1755   (Interval in Earth days: 99)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.53

137.

29.8

-7.89

32.3

48.7

Possible Mud Volcanoes Located in Acidalia Planitia:   ESP_024227_2240   ESP_024359_2240   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.66

318.

23.1

-2.47

48.5

48.7

Valleys on Western Hecates Tholus:   ESP_024207_2130   ESP_024352_2130   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.52

149.

-0.4

16.28

43.3

41.0


  


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